CWNU 3170

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0.25 UTI
0.32
CN
0.19
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 32
Radius (P>50% members) 3.3 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.19 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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CWNU 3170 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.
Very distant High extinction Very young

Data
🔍 Search references for CWNU 3170 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 29.726 66.729 0.167 -1.238 0.302 –
He et al. 2023 29.767 66.728 0.167 -1.233 0.314 –

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfr BSS
He et al. 2023 6.46 4.00 – 10 – – – –

Visualization
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CWNU 3170 UCC
Galactocentric position diagram